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How Many Black Holes Are in the Universe? 40,000,000,000,000,000,000 - SciTechDaily
Jan 19, 2022 2 mins, 48 secs
Moreover, according to their work, around 1% of the overall ordinary (baryonic) matter is locked up in stellar mass black holes.

In the first paper of a series just published in The Astrophysical Journal, the authors have investigated the demographics of stellar mass black holes, which are black holes with masses between a few to some hundred solar masses, that originated at the end of the life of massive stars.

“The innovative character of this work is in the coupling of a detailed model of stellar and binary evolution with advanced recipes for star formation and metal enrichment in individual galaxies.

This is one of the first, and one of the most robust, ab initio computation of the stellar black hole mass function across cosmic history.” — Alex Sicilia, first author of the study.

According to the new research, a remarkable amount around 1% of the overall ordinary (baryonic) matter of the Universe is locked up in stellar mass black holes.

Astonishingly, the researchers have found that the number of black holes within the observable Universe (a sphere of diameter around 90 billion light-years) at present time is about 40 billion billion (i.e., about 40 x 1018, i.e. 4 followed by 19 zeros!).

As the authors of the research explain: “This important result has been obtained thanks to an original approach which combines the state-of-the-art stellar and binary evolution code SEVN developed by SISSA researcher Dr.

Mario Spera to empirical prescriptions for relevant physical properties of galaxies, especially the rate of star formation, the amount of stellar mass and the metallicity of the interstellar medium (which are all important elements to define the number and the masses of stellar black holes).

Exploiting these crucial ingredients in a self-consistent approach, thanks to their new computation approach, the researchers have then derived the number of stellar black holes and their mass distribution across the whole history of the Universe.

Alex Sicilia, first author of the study, comments: “The innovative character of this work is in the coupling of a detailed model of stellar and binary evolution with advanced recipes for star formation and metal enrichment in individual galaxies.

This is one of the first, and one of the most robust, ab initio computation of the stellar black hole mass function across cosmic history.”.

The estimate of the number of black holes in the observable Universe is not the only issue investigated by the scientists in this piece of research.

Michela Mapelli from University of Padova, they have also explored the various formation channels for black holes of different masses, like isolated stars, binary systems, and stellar clusters.

Specifically, the researchers have shown that such events are required to explain the mass function of coalescing black holes as estimated from gravitational wave observations by the LIGO/Virgo collaboration.

in Astrophysics and Cosmology at SISSA, adds: “This research is really multidisciplinary, covering aspects of, and requiring expertise in stellar astrophysics, galaxy formation and evolution, gravitational wave and multi-messenger astrophysics; as such it needs collaborative efforts from various members of the SISSA Astrophysics and Cosmology group, and a strong networking with external collaborators.”.

training to 13 early stage researchers in the area of black hole formation and evolution, by exploiting advanced data science techniques.

Reference: “The Black Hole Mass Function Across Cosmic Times.

The Universe is a black hole filled with Electric Magnet Plasma

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